We present results from a high-resolution wide-field imaging observation of the Central Molecular Zone (CMZ) in H^13^CO^+^ J=1-0 and SiO v=0, J=2-1 emission lines using the 45-m telescope at the Nobeyama Radio Observatory in order to depict the high-density molecular gas mass distribution and explore molecular gas affected by interstellar shocks. By using the clumpfind algorithm we identify 114 molecular clumps in the H^13^CO^+^ data cube.

Cone search capability for table J/PASJ/67/90/table3 (Identified molecular clumps in the Central Molecular Zone)

Cone search capability for table J/PASJ/67/90/table4 (Expanding molecular shells in the Sagittarius B2 molecular cloud complex)